Imagen de Portada

Damping Obliquities of Hot Jupiter Hosts by Resonance Locking

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Zanazzi, J. J., Dewberry, Janosz, Chiang, Eugene
Formato:	Preprint
Publicado:	2024
Materias:	Earth and Planetary Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Spin and Obliquity Evolution of Hot Jupiter Hosts from Resonance Locks
por: Zanazzi, J. J., et al.
Publicado: (2024)

Tidal synchronization trapping in stars and planets with convective envelopes
por: Dewberry, Janosz W.
Publicado: (2024)

Tidally driven inertial waves enhance eccentricity damping and spin evolution in planets and stars
por: Dewberry, Janosz W.
Publicado: (2025)

Seismic Oscillations Excited by Giant Impacts in Directly-Imaged Giant Planets
por: Zanazzi, J. J., et al.
Publicado: (2025)

Aligned Stellar Obliquities for Two Hot Jupiter-hosting M Dwarfs Revealed by MAROON-X: Implications for Hot Jupiter Formation
por: Weisserman, Drew, et al.
Publicado: (2025)

Tidal migration of exoplanets around M-dwarfs: frequency-dependent tidal dissipation
por: Wu, Samantha C., et al.
Publicado: (2023)

TESS Giants Transiting Giants. VI. Newly Discovered Hot Jupiters Provide Evidence for Efficient Obliquity Damping after the Main Sequence
por: Saunders, Nicholas, et al.
Publicado: (2024)

Isolating the gravitational influence of Uranus's winds requires close passages inward of the rings
por: Mankovich, Christopher R., et al.
Publicado: (2025)

Saturn's Evolutionary History and Seismology: Survival of Deep Stably Stratified Regions in Evolutionary Models of Saturn Consistent with Ring Seismology
por: Su, Yubo, et al.
Publicado: (2026)

On Hot Jupiters and Stellar Clustering: The Role of Host Star Demographics
por: Kontiainen, Mika V., et al.
Publicado: (2025)

Obliquities of Exoplanet Host Stars: 19 New and Updated Measurements, and Trends in the Sample of 205 Measurements
por: Knudstrup, Emil, et al.
Publicado: (2024)

An Obliquity Measurement of the Hot Neptune TOI-1694b
por: Handley, Luke B., et al.
Publicado: (2024)

Evidence for Primordial Alignment II: Insights from Stellar Obliquity Measurements for Hot Jupiters in Compact Multiplanet Systems
por: Radzom, Brandon Thomas, et al.
Publicado: (2025)

Aligning Planet-Hosting Binaries via Dissipative Precession in Circumstellar Disks
por: Gerbig, Konstantin, et al.
Publicado: (2024)

Concealing Circumbinary Planets with Tidal Shrinkage
por: Mogan, Saahit, et al.
Publicado: (2024)

Testing the Origin of Hot Jupiters with Atmospheric Surveys
por: D'Aoust, Lina, et al.
Publicado: (2025)

Hot Jupiters are asynchronous rotators
por: Wazny, Marek, et al.
Publicado: (2024)

Hot Jupiter - Cold Jupiter: A complex sibling relation
por: Errico, Adriana, et al.
Publicado: (2026)

Eccentricities of Close Stellar Binaries
por: Wu, Yanqin, et al.
Publicado: (2024)

Geometric Considerations in Hot Jupiter Magnetic Drag Models
por: Christie, Duncan A., et al.
Publicado: (2025)

Flow Regimes in Hot Jupiter Atmospheres: Insights from Anelastic Models
por: Dietrich, W., et al.
Publicado: (2025)

Searching for Tidal Orbital Decay in Hot Jupiters
por: Alvarado III, Efrain, et al.
Publicado: (2024)

The Hot Jupiter Radius Anomaly and Stellar Connections
por: Thorngren, Daniel P.
Publicado: (2024)

Hot Jupiters are Inflated Primarily by Shallow Heating
por: Schmidt, Stephen P., et al.
Publicado: (2025)

Hot Spot Offset Variability from Magnetohydrodynamical Thermoresistive Instability in Hot Jupiters
por: Hardy, Raphaël, et al.
Publicado: (2024)

Single-Star Warm-Jupiter Systems Tend to Be Aligned, Even Around Hot Stellar Hosts: No $T_{\rm eff}-λ$ Dependency
por: Wang, Xian-Yu, et al.
Publicado: (2024)

Separating Super-Puffs vs. Hot Jupiters Among Young Puffy Planets
por: Karalis, Amalia, et al.
Publicado: (2024)

The Orbital Geometries and Stellar Obliquities of Exoplanet-Hosting Multi-Star Systems
por: Rice, Malena, et al.
Publicado: (2024)

The Resonant Remains of Broken Chains from Major and Minor Mergers
por: Li, Rixin, et al.
Publicado: (2024)

Cavitating bubbles in condensing gas as a means of forming clumps, chondrites, and planetesimals
por: Chiang, Eugene
Publicado: (2024)

Stability of Multiplanet Systems Through Hot Jupiter Destruction
por: Liveoak, Donald, et al.
Publicado: (2026)

Survival of satellites during the migration of a Hot Jupiter
por: Bolmont, Emeline, et al.
Publicado: (2025)

The Occurrence Rate of Nearby Planetary Companions to Hot Jupiters
por: Sha, Lizhou, et al.
Publicado: (2026)

Investigating the Formation of Planets Interior to in situ Hot Jupiters
por: Mathur, Devansh, et al.
Publicado: (2025)

A Hot Jupiter with a Retrograde Orbit around a Sun-like Star and a Toy Model of Hot Jupiters in Wide Binary Star Systems
por: Giacalone, Steven, et al.
Publicado: (2025)

Warm Jupiter Tidal Migration Can Spare Inner Planets; Hot Jupiter Tidal Migration May Not
por: Becker, Juliette
Publicado: (2025)

Leaning Sideways: VHS 1256-1257 b is a Super-Jupiter with a Uranus-like Obliquity
por: Poon, Michael, et al.
Publicado: (2024)

A Search for Temporal Atmospheric Variability of Kepler Hot Jupiters
por: Li, Canis, et al.
Publicado: (2024)

The role of Ohmic dissipation of internal currents on Hot Jupiter radii
por: Akgün, Taner, et al.
Publicado: (2024)

Efficiency of Hydrodynamic Atmospheric Escape in Hot Jupiters and Super Earths
por: Frelikh, Renata, et al.
Publicado: (2025)